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FluffyFriend
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where unit conventions of general relativity are used (otherwise factors of G and c would also appear). It is common to quote values of energy density directly, though still using the name "cosmological constant".
What does this paragraph mean?
I read it somewhere that a relatively newer observation renewed the concept of "cosmological constant", and it was connected with "dark energy", again, can anyone provide detailed information on that?
Wasn't "cosmological constant" proved erroneous long ago?
Or is it something are now being called "cosmological constant", something other than "cosmological constant" itself? What is it, then?
Observations announced in 1998 of distance–redshift relation for Type Ia supernovae indicated that the expansion of the universe is accelerating. When combined with measurements of the cosmic microwave background radiation these implied a value of \Omega_{\Lambda} \simeq 0.7,[5] a result which has been supported and refined by more recent measurements. There are other possible causes of an accelerating universe, such as quintessence, but the cosmological constant is in most respects the most economical solution. Thus, the current standard model of cosmology, the Lambda-CDM model, includes the cosmological constant, which is measured to be on the order of 10−35 s−2, or 10−47 GeV4, or 10−29 g/cm3,[6] or about 10−120 in reduced Planck units.
How should I understand the word "economical" here?
I know it may be quite difficult to answer my question since I got the experience when trying to explain something to an outsider about the concept withing my speciality, so I start by telling the inquisitor whatever pertinent. I'm not trying to "teach" you how to explain this issue in any fashion (if I did made you feel so, I apologize), rather, this is just a personal suggestion, because I do not even know this question I'm asking is hard to begin with or not.
I hope my question is not so valueless. Any help will be appreciated, a paragraph, a link etc. Also, sorry for my english.